Wednesday, August 25, 2021

3259 - BIG BANG - the theory as a lot to work with

  -  3258   -  BIG  BANG   -  the theory as a lot to work with.    Astronomers can observe 100 billion, billion stars similar to our Sun.  Most galaxies are still producing stars, but many galaxies have exhausted their supply of gas and can rarely produce stars.  Eventually all stars will die.



-------------------  3259  -  BIG  BANG  -  the theory as a lot to work with.    

-   Why do we think this is correct theory for the beginning of the universe?  13,700,000,000 years ago all matter and energy was the size of a dime.  The energy and matter expanded and cooled as it expanded.  Matter was created out of energy according to E = mc^2.   This equation says that matter and energy are two forms of the same thing.  Just multiply by the constant, the speed of light squared.

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-  When the cooling matched the energy of Quarks the first Quarks were formed as the building blocks for atomic nuclei.  When the Universe expanded another 1,000 times it was the size of our Solar System and the Quarks combined three at a time into protons and neutrons. 

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-  After the Universe expanded another 1,000 times the protons and neutrons combined to form hydrogen and helium nuclei.  One minute has elapsed since the Big Bang.

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-  After 300,000 years of expansion and cooling, when the Universe was 1,000 times smaller than it is today the first neutral atoms of hydrogen and helium formed as the protons captured electrons.  The photons of light were released for the first time as they escaped the ionized soup of charged particles when atoms became neutrally charged.  

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-  When the Universe expanded to 20% its present size stars and galaxies had formed.  When it was 50% its present size supernovae explosion had produced the heavy elements in the Periodic Table.  When the Universe was 67% its present size our Solar System was formed, 5,000,000,000 years ago.  In another 15,000,000,000 years the stars will all be gone.

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-  The average density in space declines as the Universe expands.  Particles uniformly fill all space as space itself expands.  Galaxies and Clusters of Galaxies are bound by gravity which is more powerful than space’s expansion at shorter distances. Space still expands between the galaxies where the force of gravity dissipates.  The force of gravity is always reduced by the square of the distance of separation.  

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-  Hubble’s law for expanding space says that the recession velocity of a galaxy is equal to the distance to the galaxy multiplied by 47,000 miles per hour per million lightyears distance.  

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-  Distant galaxies measured by their redshift due to the expanding space are moving away at greater the 90% the speed of light.  The more space there is between us the faster they are moving away.

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-  The proportions of the light elements, hydrogen, helium, lithium, and beryllium,   match well with calculations assuming the Big Bang was a giant thermonuclear reactor.  The protons and neutrons after fusion reactions would match the expanded proportions of helium4, helium3, lithium7 and deuterium2. 

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-   Today 24% of all the elements is helium4, a perfect match since helium is inert and should remain the same.  Also,  10^-4, or, 0.01%, for the element deuterium2.  And, 10^-5 for the element helium3.  And,   10^-10 proportions for the element lithium7 isotope.  The mix of these elements supports the Big Bang theory.

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-  Galaxies form because gravity causes density fluctuations in the distribution of matter.  Gravity slows the expansion of denser regions causing them to grow even more dense, in turn increasing the amount of gravity.  The fabric of galaxies laced amongst the voids of space match the expected expansion of matter and energy in the Big Bang theory.

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-  As part of this expanding Universe there is a window of time that life could form.  In an earlier Universe it was too hot.  In an older Universe it will be too cold. 

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-   Today astronomers have a lot to work with.  They can observe 100 billion, billion stars similar to our Sun.  Most galaxies are still producing stars, but many galaxies have exhausted their supply of gas and can rarely produce stars.  Eventually all stars will die.

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-   Fortunately, we have arrived in the right Cosmic time for this astronomy lesson.

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-  August 25, 2021     BIG  BANG  -   as a lot to work with?    1128       3259                                                                                                                                                     

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---   Some reviews are at:  --------------     http://jdetrick.blogspot.com -----  

--  email feedback, corrections, request for copies or Index of all reviews 

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Wednesday, August 25, 2021  ---------------------------






3258 - BLACKHOLES - explained?

  -  3258   - BLACKHOLES  -  explained?   Picture two merging galaxies and the resulting creation of Blackholes in the massive star formations that came out of the collision.  What are the conditions that create these astronomical mysteries?


-----------------------------  3258  -   BLACKHOLES  -  explained?

-  A Blackhole in astronomy is a region in space where so much mass is concentrated into so small a volume that the fabric of space-time is warped so much the space and time are effectively cut off from the rest of the Universe.  Time stops.  Space disappears into a ‘Singularity“.

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-  A Singularity is a hypothetical point in the center of the Blackhole where all the mass and space are concentrated into infinity density.  If the Blackhole is rapidly spinning than the Singularity becomes a super dense ring not a super dense point.

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-  Blackholes are common in the Universe.  “Stellar Blackholes” are created with massive supernovae that over 8 times the mass of our Sun.  “Galactic Blackholes” are a million to a billion times the mass of our Sun and exist at the centers of nearly every large galaxy that astronomers have studied. 

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-   Maybe smaller Blackholes exist as well but we have not been able to create them in our laboratories or particle accelerators to date.  Stay tuned.

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-  If we could compress the entire Earth down to less than 2 inch diameter than it would become a Blackhole.  A Blackhole is created when the mass is large and the volume is small.  

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-  The volume is always spherical, therefore, it is a function of the radius.  These two things determine the escape velocity needed to escape the immense gravity.  When the escape velocity exceeds the speed of light nothing, nothing can escape.  

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-  When the radius of the Earth is compressed to 1 inch not even light photons can leave that surface of the Blackhole that is created.  This spherical surface is called the “ Event Horizon”.

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-  Besides escape velocity, the other way to describe the Blackhole creation is that the massive gravity is so intense it warps the fabric of space-time into a closed loop.

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-  The formula for radius and mass at which this happens is:

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--------------------  R  =  2 * G * M  / c^2

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--------------------  Radius  =  2 * Gravitational Constant * Mass /  speed of light squared

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-------------------  The ratio of R /  M  =  a constant


--------------------  If two variables are proportional they can be turned into an equality with the proper Constant of Proportionality.  In this case, the constant =  2 * G / c^2

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--------------------  G  = 6.67 * 10^-11 meter^3 / kilogram* seconds^2

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--------------------  c^2  =  9 *10^16 meters^2 / seconds ^2

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-------------------  R / M  =  1.48 * 10^-27 meters / kilogram.

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-  This formula works for all sizes of Blackholes that are not spinning.  Spinning Blackholes require equations from the Theory of Relativity in order to calculate their Event Horizon as a function of mass and spin.

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-  If an average human was compressed into a Blackhole it’s size would have a radius of 10^-23 centimeters, 10 times smaller than the radius of a proton.

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-  If the Sun were compressed into the size having a 1.8 mile radius it would become a Blackhole.

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-  There was the collision of two galaxies located 430,000,000 lightyears away from us.  An Elliptical Galaxy and a Spiral Galaxy collided.  X-rays were recorded by the Chandra X-ray telescope.  

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-  The result of the collision was an expanding wave of star formation containing an abundance of massive young stars.  These massive stars many times larger than our Sun have very short lives.  The massive stars burn through their fuel in a few million years and explode in a giant supernovae.  The remnant left in the center of these supernova explosions becomes a Neutron Star, or, a Blackhole.

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-  The X-ray sources around the blue ring are so bright in X-rays that they must be Blackholes with masses 10 to 20 times that of our Sun.

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-  The Elliptical Galaxy also has a super massive Blackhole at its center.  This Blackhole is more easily identified in a purely X-ray image not blocked by the visible light.

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-  Each Blackhole has a spherical radius depending on its mass and spin.  When a massive star that is 20 Solar Mass explodes as a supernova, the remnant left behind at the center is 8 Solar Mass.  

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-  The 8 Solar Mass is compressed into such a small volume by that much gravity that is left that it compresses into a Blackhole.  The X-rays are emitted from the gasses that are orbiting the Blackhole in its spinning accretion disk.

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-  The in falling, spinning gases have colliding atoms creating enormous friction and collisions at higher and higher speeds.  This in-falling gas gets heated to over 100,000,000 Kelvin, causing the atoms to emit X-rays.  

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-  The temperature of the gas is related the distance to the Blackhole.  If the 8 Solar Mass Blackhole is non-rotating we can calculate how far away the gas atoms are from the Singularity at the center of the Blackhole.

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------------  Radius of the Event Horizon  =  3.0 * Solar Masses

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------------  Rs  =  3.0 * 8  =  24 kilometers  =  15 miles.

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-----------  Radius of the distance outside the Event Horizon where photons can orbit at the speed of light and not fall into the Blackhole  =  1.5 * Rs

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----------- Radius  =  1.5 * 24  =  36 kilometers  =  22 miles.

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-----------  Radius of the distance outside the Event Horizon where material particles can orbit and not fall into the Blackhole  =  3.0 * Rs

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-----------  Radius  =  3 * 24  =  72 kilometers  =  45 miles.

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-  So, you can see that a Stellar Blackhole that is only 8 Solar Mass is not very big.  The part we can see is only 100 miles in diameter.  Of course, the Galactic Blackholes are much bigger.  The Milky Way Blackhole is 4,000,000 Solar Mass.  The Andromeda Galaxy Blackhole is 140,000,000 Solar Mass.  

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-  Over 1 million Quasars have been identified.  These are giant galaxies with giant Blackholes with masses in the billions of Solar Mass.  These Quasars are so big they burn their fuel in a very short time, 100 million years.  

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-  Some that astronomers have found are over 13 billion lightyears away.  The accretion disks and the corresponding jets are so bright that they totally outshine the entire galaxies they are in. 

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-   What we are seeing happened 13,000,000,000 years ago.  I wonder what they look like today?  Did they continue to grow?  Or, did they evaporate and die?  To learn more:

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----------   I also have some other Reviews on Blackholes, available upon request:

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-  1105  -  How Small Can Blackholes Get?

-  1177  -  Blackholes in Astronomy

-  1096  -  Are Blackholes Monsters or Creators?

-  903  -  Spinning Blackholes.

-  848  -  Blackholes are Everywhere.

-  2380  -  Too Weird to Ponder

-  819  -  Blackhole of All Sizes.

-  774  -  Seeing Blackholes.

-  580  -  Blackholes

-  453  -  Blackholes are Neither

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-  August 23, 2021      BLACKHOLES  -  explained?          1244        3258                                                                                                                                                      

----------------------------------------------------------------------------------------

-----  Comments appreciated and Pass it on to whomever is interested. ---- 

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com -----  

--  email feedback, corrections, request for copies or Index of all reviews 

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Wednesday, August 25, 2021  ---------------------------






Monday, August 23, 2021

3257 - NEUTRON STARS - collapse from white dwarfs?

  -  3257    -   NEUTRON  STARS  -  collapse from white dwarfs?    A nearby White Dwarf star found in 2021 might be about to collapse into a Neutron Star.  About 97% of all stars in our Universe are destined to end their lives as “white dwarf stars“, which represents the final stage in their evolution. 


--------------  3257  -  NEUTRON  STARS  -  collapse from white dwarfs?

-  Like neutron stars, white dwarfs form after stars have exhausted their nuclear fuel and undergo gravitational collapse, shedding their outer layers to become super-compact stellar remnants. This will be the fate of our Sun billions of years from now, which will swell up to become a “red giant star” before losing its outer layers.

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- Unlike neutron stars, which result from the more massive stars, white dwarfs were once about eight times the mass of our Sun or lighter. ( 8 Solar Mass).  The density and gravitational force of these objects is an opportunity to study the laws of physics under some of the most extreme conditions imaginable. 

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-  One such object has been found that is both the smallest and most massive white dwarf ever seen.    This white dwarf, known as “ZTF J190132.9+145808.7” is located about 130 light-years from Earth and is estimated to be 1.35 times as massive as our Sun.

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-   This white dwarf star has a stellar radius of about 1,125 miles, which is slightly larger than our Moon 1,080 miles, making it the smallest and most massive white dwarf we have ever observed. 

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-  It may seem counterintuitive, but smaller white dwarfs happen to be more massive. This is due to the fact that white dwarfs lack the nuclear burning that keep up normal stars against their own self gravity, and their size is instead regulated by “quantum mechanics.”

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-  This white dwarf also has an extreme magnetic field, ranging from 600 to 900 MegaGauss over its entire surface, or roughly 1 billion times stronger than our Sun’s. This magnetic field has one of the fastest rotational periods ever observed in an isolated white dwarf, whipping around the star’s axis once every 6.94 minutes.  That is fast spinning!

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-  Spectra obtained by “Keck’s Low-Resolution Imaging Spectrometer” (LRIS) revealed signatures of a powerful magnetic field, ultraviolet data from “Swift  observatory” helped constrain the size and mass of the white dwarf.

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-  Between its strong magnetic field and seven-minute rotational speed this white dwarf must be the result of two smaller white dwarfs coalescing into one. Roughly 50% of the stars in the observable Universe are binary systems, consisting of two stellar companions that orbit one other. If these stars are less than eight solar masses each, they will evolve into white dwarfs that eventually merge to form a more massive white dwarf star.

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-  This process boosts the magnetic field of the resulting white dwarf and speeds up its rotation compared to that of its progenitors. It would also explain how this star manages to concentrate such a considerable mass into a volume slightly more than that of the Moon. 

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-   It’s possible that this white dwarf is massive enough to further collapse into a neutron star. It is so massive and dense that, in its core, electrons are being captured by protons in nuclei to form neutrons. Because the pressure from electrons pushes against the force of gravity, keeping the star intact, the core collapses when a large enough number of electrons are removed.

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-  It may mean that a significant portion of other neutron stars in our galaxy did not start their lives as massive stars, but instead evolved from smaller binary stars. The newfound object’s close proximity to Earth (130 light-years) and the fact that it is relatively young (100 million years old ) are indications that similar objects could be common in our galaxy.

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-   Scientists hope to be able to study the population of white dwarfs as a whole and determine how many were the result of massive stars experiencing a supernova, and how many were the result of binary companions merging near the end of their lives.

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-  They hope to learn the rate of white dwarf mergers in the galaxy, and is it enough to explain the number of type 1a supernovae?


-   How is a magnetic field generated in these powerful events, and why is there such diversity in magnetic field strengths among white dwarfs?

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-   Finding a large population of white dwarfs born from mergers will help us answer all these questions and more.  The more we learn the more we don’t know!

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-  August 23, 2021       NEUTRON  STARS  -  collapse from white dwarfs?        3257                                                                                                                                                      

----------------------------------------------------------------------------------------

-----  Comments appreciated and Pass it on to whomever is interested. ---- 

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com -----  

--  email feedback, corrections, request for copies or Index of all reviews 

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Monday, August 23, 2021  ---------------------------






3256 - STARS - in our solar system?

  -  3256   -  STARS  -  in our solar system?   Every 50,000 years or so, a nomadic star passes near our solar system. Most brush by without incident. But, every once in a while, one comes so close that it gains a prominent place in Earth’s night sky, as well as knocks distant comets loose from their orbits.



-----------------------------  3256  -  STARS  -  in our solar system?

-  Wandering stars pass through our solar system surprisingly often. Our Sun, which is our closest star, has had close encounters with other stars in the past, and it’s due for a dangerously close one in the not-so-distant future.

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-  The most famous of these stellar interlopers is called “Scholz’s Star“. This small binary star system was discovered in 2013. Its orbital path indicated that, about 70,000 years ago, it passed through the Oort Cloud, the extended sphere of icy bodies that surrounds the fringes of our solar system. 

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-   Some astronomers even think Scholz’s Star could have sent some of these objects tumbling into the inner solar system when it passed.  However, Scholz’s Star is relatively small and rapidly moving, which should have minimized its effect on the solar system. 

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-  Scientists have been finding that these kinds of encounters happen far more often than once expected. Scholz’s Star wasn’t the first flyby, and it won’t be the last. In fact, we’re on track for a much more dramatic close encounter in the not-too-distant future.

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-   Since this star didn’t appear to be moving much side to side, the star was likely moving toward us or away from us at a breathtaking pace. As the astronomers measured the star’s radial velocity to learn how quickly it was moving toward or away from our Sun.  The initial results that this thing came within one parsec [3.26 light-years] of the Sun.

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-  It passed closer to our Sun than any other known star. Another wandering star passed within one light-year of the Sun roughly 70,000 years ago. At the time, modern humans were just beginning to migrate out of Africa, and Neanderthals were still sharing the planet with us.

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-   The European Space Agency satellite called “Gaia“, is built to map the precise locations and movements of over a billion stars, and we now know about other close encounters.  In 2018, a team of researchers  used Gaia data to plot our Sun’s future meet-ups with other stars. 

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-  They discovered nearly 700 stars that will pass within 15 light-years of our solar system over just the next 15 million years. However, the vast majority of close encounters have yet to be discovered. But they suspect roughly 20 stars should pass within just a couple light-years of us every million years.

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-  Space is big.  Statistically, most of those stars would pass the outer edge of our solar system. That means encounters like the one with Scholz’s Star are common, but only a few are close enough to actually dislodge a significant number of comets,

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-  A few stars should still come surprisingly close. And if a large, slow-moving star did pass through the edge of the Oort Cloud, it could really shake up the solar system.

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-  Many nearby stars will pass close to the Oort Cloud, but only one will move through it. In about 1.35 million years, “Gliese 710” likely will gravitationally perturb millions of comets, sending a sizable number on a potential collision course with Earth.

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- A massive star steamrolling through the outer solar system is exactly what Gaia data show will happen less than 1.4 million years from now, according to a 2016 study. 

The star called Gliese 710 will pass within 10,000 astronomical units.

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-  1 AU is equal to the average Earth-Sun distance of 93 million miles. 10,000 AU is well within the outer edge of the Oort Cloud.

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-   At half the mass of the Sun, Gliese 710 is much larger than Scholz’s Star, which is just 15 percent the mass of the Sun. This means Gliese 710’s hulking gravity could potentially wreak havoc on the orbits of icy bodies in the Oort Cloud.

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-   While Scholz’s Star was so tiny it would have been barely visible in the night sky, Gliese 710 is larger than our current closest neighbor, Proxima Centauri. So when Gliese 710 reaches its closest point to Earth, it will burn as a brilliant orange orb that will outshine every other star in our night sky.

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-  This event could be “the strongest disrupting encounter in the future and history of the solar system.  Fortunately, the inner solar system is a relatively tiny target, and even if Gliese 710 does send comets flying our way, it would take millions of additional years for these icy bodies to reach us. That should give any surviving future humans plenty of time to take action.  Yeah right, if we could just stop fighting each other!

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-  And in the meantime, they can enjoy watching what may be one of the closest stellar flybys in the history of our solar system.

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-  How do we discover these wandering comets?  Sometimes the old methods  are the best methods. When astronomer Clyde Tombaugh discovered Pluto in 1930, it was the result of countless hours spent straining his eyes at a machine called a “blink comparator“. Using it, Tombaugh could flip rapidly back and forth between two images of the night sky taken at slightly different times.

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-  Volunteers comb through images of our celestial neighborhood, looking for new worlds near to us, just like Tombaugh. But instead of planets, they’re now looking for something even stranger. The search today is focused on a strange class of objects known as “brown dwarfs“,  Sized to be not quite planets, not quite stars.

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-   Scientists involved with the project have now released the most up-to-date map yet of brown dwarfs stars near Earth, something they say wouldn’t have been possible without the hard work of citizen scientists. 

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-  The map will help astronomers better understand how brown dwarfs form and evolve, and give researchers a better idea of the objects that populate the space just beyond our own solar system. Their research was published online in late 2020.

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-   February 18, 1930, Tombaugh was flipping through recent images when he noticed a tiny dot that jumped back and forth, a sign that he’d found a nearby object. Further observational work ruled out other objects like asteroids, and the discovery of the onetime ninth planet was official. Today, Pluto has been demoted to the status of dwarf planet as we’ve discovered other objects like it in the Solar System.

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-   Astronomers have strong suspicions that we’re not yet done discovering worlds in the outer reaches of the Solar System quite yet. A number of minor planets and other so-called “Kuiper Belt objects” have been discovered in recent years. And some astronomers think there’s another large planet orbiting far out beyond Neptune, which they call “Planet Nine.”

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-  Even further out in our celestial neighborhood there are likely to be a number of dim, mysterious objects known as brown dwarfs. Too large to be planets but not large enough to be stars, brown dwarfs are a strange kind of in-between object. They’re typically defined as being somewhere between 13 and 80 times the mass of Jupiter. 

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-  The updated map includes 525 brown dwarfs within 65 light-years of Earth, but more are surely waiting out there.  Brown dwarfs are very hard to find.  Because they aren’t big enough to begin fusing hydrogen into helium, the process that powers our Sun and other stars,  brown dwarfs are often quite cool, meaning they don’t emit a lot of radiation that astronomers can pick up on. 

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-  Astronomers have found a wide variety of brown dwarfs that differ in terms of composition and internal activity. Still, many questions remain about how brown dwarfs form and what they look like. More observations are needed to get to the bottom of the mystery.

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-  That’s where citizen science comes in. Astronomers already have access to broad, high-resolution photos of nearly the entire night sky from data gathered from NASA’s Wide-field Infrared Survey Explorer, or WISE, spacecraft. Beginning in 2009, the satellite scanned the heavens in various infrared frequencies, and a second phase, dubbed NEOWISE, began in 2013.

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-  Astronomers planned to follow up on anything interesting they spotted in the WISE images with other, more powerful infrared telescopes like the Spitzer Space Telescope. But they soon ran into a big problem: NASA was planning on shutting Spitzer down. To find anything, the scientists would need to move quickly.

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-   Volunteers use an online tool to quickly flip through images of the night sky taken a short time apart. If they spot something moving, they’re able to alert astronomers, who’ll follow up on their work with more powerful observations using observatories. 

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-  Volunteers found dozens of new brown dwarfs candidates that scientists were able to follow up on with Spitzer to help create the new map. In all, the citizen scientists helped add 52 new brown dwarfs in just a year.

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-  Though Spitzer shut down in January of 2020, the astronomers were able to follow up on many promising candidates citizen scientists picked out. This led to the discovery of, among other things, a new class of brown dwarf, called extreme “T-type sub dwarfs“. 

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-  These objects are extremely old, in some cases around 10 billion years old, scientists. Other unique observations from the new map include the coldest known brown dwarf, a place where temperatures probably dip below the freezing point.

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-  One of the citizen scientists did find a really, really faint object that was just streaking across the sky. And we thought, ‘What is this? This is going to be something weird. The object didn’t match the spectrums of anything they had on file.  Further findings showed it was a very ancient cold brown dwarf composed largely of hydrogen, without the metals most other brown dwarfs have.

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-  One volunteer even coded a tool, known as WiseView, that makes the process of discovering brown dwarfs far easier by allowing participants to flip easily back forth through the images.

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-Volunteers are invited to listen in on weekly telephone meetings between the scientists as well, where they discuss recent results and new objects to focus on.

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-  To join in with citizen scientists across the world, and to get a little taste of how Clyde Tombaugh found Pluto, head to the Backyard Worlds project affiliate page on SciStarter. In your SciStarter dashboard, add your Zooniverse name under "Info & Settings" to earn credit for your participation. And maybe you’ll even find your own world, floating out there in space.

-  August 22, 2021         STARS  -  in our solar system?                     3256                                                                                                                                                      

----------------------------------------------------------------------------------------

-----  Comments appreciated and Pass it on to whomever is interested. ---- 

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com -----  

--  email feedback, corrections, request for copies or Index of all reviews 

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Monday, August 23, 2021  ---------------------------






Sunday, August 22, 2021

3255 - MASS - creating matter from light?

  -  3255   -  MASS  -  creating matter from light?     Einstein’s 1905 paper speculated about the excess energy might be balanced by a loss of mass of the nuclear particles. This idea eventually led to Einstein’s most famous equation, E = mc2.  Energy and mass are two forms of the same thing?


 ------------------  3255  -  MASS  -  creating matter from light?              

-  In 1905 Albert Einstein wrote four groundbreaking papers on quantum theory and relativity.  One was on “brownian motion“, one earned him the Nobel prize in 1921, and one outlined the foundations of special relativity. But it’s Einstein’s last 1905 paper that is the most unexpected.

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-  The paper is just two pages long, and it outlines how “special relativity” might explain a strange aspect of radioactive decay. As Marie Curie most famously demonstrated, some materials such as radium salts can emit particles with much more energy than is possible from simple chemistry. 

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-  This equation is often taken to mean that matter and energy are two sides of the same coin. It actually means that the apparent mass and energy of an object depend upon the relative motion of an observer, and because of this, the two are intertwined, similar to the connection between space and time.   Spacetime…. MasssEnergy!

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-  One consequence of this relation is that under the right circumstances objects should be able to produce energy via a loss of mass.

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-  We now know this is exactly what happens in radioactive decay. The effect is also how stars create energy in their cores via nuclear fusion. Of course, if matter can become energy, then it should also be possible for energy to become matter.

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-   It took the invention of particle accelerators to pull this off.   Accelerate particles to nearly the speed of light and slam them together. The large apparent mass of the particles releases tremendous energy, and some of that energy changes back into particles. All of this modern particle physics can trace its history to Einstein’s two-page paper.

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-  The laws of physics don’t just say you can create energy from matter and vice versa, it places specific constraints on the nature of the created matter and energy. 

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-  One of the simplest examples of this is “electron-positron annihilation“. This happens when an electron collides with its antimatter twin, the anti-electron, called a positron. The two particles have the same mass, but opposite charge, so when they collide they produce two high-energy photons. The mass of the electron and positron are transformed entirely into energy. This experiment was first proposed in the 1930s, but it wasn’t done until 1970.

-

-  If you can convert matter entirely into energy, you should be able to do the reverse. It’s known as the “Breit–Wheeler process” and involves colliding two photons to create an electron-positron pair. While we have used light to create matter several times, converting two photons directly into matter is very difficult. But a recent experiment shows it can be done.

-

-  The team used data from the Relativistic Heavy Ion Collider (RHIC) and looked at more than 6,000 events that created electron-positron pairs. They didn’t simply beam two lasers at each other but instead used high-energy particle collisions to create intense bursts of photons. In some cases, these photons collided to create an electron-positron pair. From the data, they could show when a pair was created directly from light.

-

-  Since these pair productions occurred in the intense magnetic field the team also demonstrated another interesting effect known as “vacuum birefringence“. Normal birefringence occurs when light is split into two beams of different polarization. This effect occurs naturally in materials such as “Iceland spar“. 

-

-  With vacuum birefringence, light passing through an intense magnetic field is split into two polarizations, with each polarization taking a slightly different path. It’s an amazing effect if you think about it because it means you can change the path of light in a vacuum, using only a magnetic field. Vacuum birefringence has been observed in the light coming from a neutron star, but this is the first time in 2021 it’s been observed in the lab.  What next?

-

-  August 20, 2021       MASS  -  creating matter from light?              3255                                                                                                                                                      

----------------------------------------------------------------------------------------

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--------------------- ---  Sunday, August 22, 2021  ---------------------------






Friday, August 20, 2021

3254 - COMET - largest one found?

  -  3254   -  COMET  -  largest one found?   A giant comet was found far out in the solar system.  It may be 1,000 times more massive than a typical comet, making it potentially the largest ever found in modern times.  Called Comet C/2014 UN271 or Bernardinelli-Bernstein after its discoverers.


 ------------------  3254  -  COMET  -  largest one found?

-  Astronomers estimate this icy comet has a diameter of 62 miles to 124 miles , making it about 10 times wider than a typical comet. This estimate is quite rough as the comet remains far away from Earth and its size was calculated based on how much sunlight it reflects.

-

-   The comet will make its closest approach to our planet in 2031 but will remain at quite a distance even then.  I hope my grandkids are watching?  Astronomers have found this comet early enough for them to watch it evolve as it approaches and warms up.

-

-   The comet was first spotted in archival images from the “Dark Energy Survey” taken in 2014.  The comet is now located at the equivalent distance of Uranus, roughly 20 astronomical units (AU) from the sun.

-

 -  (One AU is the Earth-sun distance, about 93 million miles, or 150 million kilometers). 

-

-  The comet shines at magnitude 20, making it out of reach of most amateur astronomers' telescopes.  Most amateur star watchers can see objects of magnitude 5 or 6 with the naked eye in dark conditions.

-

- When the comet swings closer to Earth in 2031, it will still be at 11 AU, which is a little more distant than Saturn's average orbit from the sun. Even then, amateur sky watchers will still need to use very large telescopes to see it.

-

-  What makes this comet  so special, aside from its size, is the fact it hasn't visited the inner solar system in three million years, roughly the same era that the famous human ancestor "Lucy" was walking the Earth. 

-

-  The comet originated some 40,000 AU away from the sun in the Oort Cloud, which is a huge, distant region of space thought to hold trillions of comets.

-

-  The comet popped up during a scan of archival images of the Dark Energy Survey, which uses a wide-field 570-megapixel CCD imager mounted on the Víctor M. Blanco 4-meter telescope at Cerro Tololo Inter-American Observatory in Chile.

-

- This survey's main goal is mapping 300 million galaxies across a swath of the night sky, but its deep-sky observations have also yielded several comets and “trans-Neptunian objects” (TNOs), which are icy worlds orbiting beyond Neptune.

-

-  The comet was spotted using the National Center for Supercomputing Applications and Fermilab, identifying 800 TNOs from archival survey data. While the images of the comet didn't show a classic tail between 2014 and 2018, an independent observation from the Las Cumbres Observatory network in 2021 showed the comet now has a coma of gas and dust surrounding it.

-

-  The image from the “Dark Energy Survey” (DES) is composed of some of the discovery exposures collected by the 570-megapixel Dark Energy Camera (DECam) mounted on the Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory (CTIO) in Chile. The image shows the comet in October 2017, when it was 25 astronomical units away, 83% of the distance to Neptune.

-

-  Studying the comet will not only give us more insight into how this massive object formed and evolves, but it also could shed light on the early history of giant planet movements in the solar system. 

-

-   Astronomers suspect that there may be many more undiscovered comets of this size waiting in the Oort Cloud far beyond Pluto and the Kuiper Belt.  These giant comets are thought to have been scattered to the far reaches of the solar system by the migration of Jupiter, Saturn, Uranus and Neptune early in their our Solar System history.

-

-  It's harder to predict if any spacecraft will be able to observe the comet's approach, because space missions tend to be shorter than the lifespans of ground-based scopes. It's possible, however, that a future telescope or mission could be funded by 2031 for comet observations that is not yet approved or even planned.

-

-   The major space agencies may also task existing spacecraft across the solar system to look at Comet Bernardinelli-Bernstein, as happened near Mars in 2014 when Comet Siding-Spring zoomed past the Red Planet.

-

-  NASA's James Webb Space Telescope is scheduled to launch in late 2021 for a prime mission of at least 5 1/2 years, although Webb could run for a decade or more if it remains healthy and funding is maintained.

-

-   The Hubble Space Telescope is famous for comet observations and may be available in 2031, although predictions say it could be healthy through the mid-2020s and will be deorbited no later than the 2030s.

-

-  August 20, 2021       COMET  -  largest one found?                      3254                                                                                                                                                      

----------------------------------------------------------------------------------------

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---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Friday, August 20, 2021  ---------------------------






3253 - MOON - the total eclipse in 2010

  -  3253   -  MOON  -  the total eclipse in 2010.  We tend to take the Moon for granted.  We know it circles the Earth every month and there are phases of the Moon from New Moon to Full Moon.  But the Full Moon does not occur the same day every month.  That is because the Moon’s orbit is once every 27.55 days.  That does not match up exactly with our 30 and 31 day months.  In fact, once in a Blue Moon we have two Full Moons in the same month.  The devil is in the details.


 ------------------  3253  -  MOON  -  the total eclipse in 2010

-  The Moon contains some interesting facts that make for conversation at your next  Moon party.  The total eclipse of the Full Moon had occurred on Monday night at midnight, December 20, 2010.

-

-  If you had a party you may have used some trivia to keep things lively because it takes 1 ½ hours for the Earth’s shadow to cross the Moon.   

-

-   The Full Moon looks very bright in the night sky.  It is a mirror for the bright sunlight that is coming from behind us.  However, the Moon is only reflecting 7% of the sunshine that strikes its surface.  By comparison the Earth reflects 37% of the sunlight. 

-

-   A Full Earth would be 5 times brighter then the Full Moon.  The Sun would be 450,000 times brighter.  The Full Moon appears brightest when it is directly overhead at midnight.  That is because it is a few percent closer and you are viewing it through less atmosphere, as much as 13% less depending on the angle you are viewing toward the horizon.  It also appears brighter when the air is dry.  Water vapor will scatter the moonshine making it appear dimmer.

-

-  With a telescope or binoculars you can easily resolve on arc second on the Moon.  One arc second on the Moon’s surface corresponds to 1 mile of resolution.  The diameter of the Moon is 1800 arc seconds.  This is ½ degree in diameter the same as the Sun.  

-

-  You can see over 30,000 craters on the Moon, if you have time to count them.  By comparison the Earth has about 200 visible craters.

-

-  The Moon does not orbit the center of the Earth.  The Earth and the Moon share a common center of gravity.  That spot is 1,000 miles below your feet when the Moon is directly overhead.  This spot is still 2,900 miles above the center of the Earth.

-

-  The Moon has a circular orbit that turns slightly more elliptical during a New Moon and a Full Moon.  That elliptical shape rotates around the Earth completing a cycle every 9 years.  As a consequence of this elliptical rotation the Moon never returns to the same starting point after each orbit.  If you were in outer space and tracing out the Moon’s orbit about the Earth the tracing would look like the petals of a daisy.

-

-  The Moon moves through the sky its own diameter every hour, going west to east.  It is traveling 2,237 miles per hour and its diameter is 2,160 miles. So, it travels its own diameter every hour.  This makes it easy to predict where it will be a few hours later in the sky.

-

-  The Earth has a 23 ½ degree tilt compared to the plane of the orbits of the other planets.  The Moon chooses to orbit with the other planets and not with the Earth.  The Moon does not orbit the equator of the Earth.  That is the reason that its path, which is near the elliptic, is higher and lower on the horizon much like the Sun and the other planets. 

-

-   However, the Moon does not stay on this perfect plane.  Again it wobbles.  It completes one wobble every 18.61 years and the tilt of the wobble is up to 5 degrees.  Looking at the Moon and the Sun-Earth plane from outer space the Moon’s orbit would trace out a wobble like a dropped dish rattling on the floor.

-

-  This wobble results in the Full Moon being 5% higher in the night sky at certain times of the 19 year cycle.  On the 21st of December, 2010, the Full Moon is the highest it gets in the sky of that year.  At 12:01 A.M. on the 21st the total eclipse will begin replacing the 120 stars you can see in the sky with 2,600 stars as the darkness brings them out. 

-

-  The angular size of the Moon in the sky varies from 25 arc minutes to 27 arc minutes during the month.  We tend to estimate that at ½ degree.  It is one of the largest moons in the Solar System.  4 others are larger, but, our Moon is larger than the wannabe planet Pluto.  The Moon is 27% the size of the Earth in diameter.  Few people believe that when they first learn that the Moon is ¼th the size of the Earth.

-  August 18, 2021       MOON  -  facts to amaze you?          1232      3253                                                                                                                                                      

----------------------------------------------------------------------------------------

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---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Friday, August 20, 2021  ---------------------------






Thursday, August 19, 2021

3252 - UNIVERSE - how much does it weigh?

  -  3252   -   UNIVERSE  -  how much does it weigh?  By combining  measurements using different techniques, astronomers were able to determine a best combined value, concluding that matter makes up 31.5±1.3% of the total amount of matter /  energy in the universe. Only 5% is “Normal Matter”.  You , me, and everything we see.  


 ------------------  3252  -  UNIVERSE  -  how much does it weigh?

-   How can we possible precisely measure the total amount of matter in the universe?   A  daunting exercise.   

-

-  Astronomers determined that matter makes up 31% of the total amount of matter and energy in the universe, with the remainder, 69%, consisting of “dark energy“.

-

-  If all the matter in the universe were spread out evenly across space, it would correspond to an average mass density equal to only about six hydrogen atoms per cubic meter.

-

-  However, since we know 80% of matter is actually “dark matter“, in reality, most of this matter consists not of hydrogen atoms but rather of a type of matter which cosmologists don't yet understand.  You kids are going to have to figure this out for yourselves.  We don’t get it?

-

-  The technique for determining the total amount of matter in the universe is to compare the observed number and mass of galaxy clusters per unit volume with these predictions from  simulations.

-

-   Because present-day galaxy clusters have formed from matter that has collapsed over billions of years under its own gravity, the number of clusters observed at the present time is very sensitive to the total amount of matter that exists.

-

-  A higher percentage of matter would result in more galaxy clusters.  "The 'Goldilocks'“ challenge for our team was to measure the number of clusters and then determine which answer was 'just right.'   But it is difficult to measure the mass of any galaxy cluster accurately because most of the matter is “dark” so we can't see it with telescopes.

-

-  To overcome this difficulty, astronomers developed "GalWeight," a cosmological tool to measure the mass of a galaxy cluster using the orbits of its member galaxies. The Sloan Digital Sky Survey (SDSS) was used to create "GalWCat19," a publicly available catalog of galaxy clusters. 

-

-  Then they compared the number of clusters in their new catalog with simulations to determine the total amount of matter in the universe.

-

-  This is the first use of the galaxy orbit technique which has obtained a value in agreement with those obtained by teams who used noncluster techniques such as “cosmic microwave background anisotropies“, “baryon acoustic oscillations“, “Type 1a supernovae“, and “gravitational lensing."


-   Using the  GalWeight galaxy orbit technique astronomers were able to determine a mass for each cluster individually rather than rely on more indirect, statistical methods.

-

-  By combining these measurements with those from the other teams that used different techniques, they were able to determine a best combined value, concluding that:

-

----------------------------  Matter makes up 31.5±1.3% of the total amount of matter /  energy in the universe.

-

-  I thought you needed to know that.  Only 5% is “normal matter“.  I left the rest for you to figure out.  You can convert these percentages to pounds or kilograms if you like.

-

-  August 18, 2021     UNIVERSE  -  how much does it weigh?           3252                                                                                                                                                      

----------------------------------------------------------------------------------------

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--  email feedback, corrections, request for copies or Index of all reviews 

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Thursday, August 19, 2021  ---------------------------






Wednesday, August 18, 2021

3251 - CURIOSITY - the rover on Mars?

  -  3251   -   CURIOSITY  - the rover on Mars?    It is hard for me to believe.  But we still have robots roaming around the surface of Mars.  Images of knobbly rocks and rounded hills are being sent to us by “Curiosity rover” after it climbed Mount Sharp, a 5-mile-tall mountain within the 96-mile-wide basin of Mars' Gale Crater.


 ------------------  3251  -  CURIOSITY  - the rover on Mars?

- The Curiosity rover's Mast Camera, or Mastcam, highlights those features in a panorama captured on July 3, 2021 (the 3,167  Martian day, or sol, of the mission).

-

-  Spacecraft orbiting Mars show that Curiosity is now somewhere between a region enriched with clay minerals and one dominated by salty minerals called sulfates. The mountain's layers in this area may reveal how the ancient environment within Gale Crater dried up over time. Similar changes are seen across the planet, and studying this region up close has been a major long-term goal for the mission.

-

-  The rocks in this crater begin to tell us how this once-wet planet changed into the dry Mars of today, and how long habitable environments persisted even after that happened.

-

-  Curiosity landed nine years ago, on August 5, 2012 PDT , to study whether different Martian environments could have supported microbial life in the planet's ancient past, when lakes and groundwater existed within Gale Crater.

-

-  The rover pulverizes rock samples with a drill on its robotic arm, then sprinkles the powder into the rover's chassis, where a pair of instruments determines which chemicals and minerals are present.

-

-   Curiosity recently drilled its 32nd rock sample, as of 2021, from a target nicknamed "Pontours" that will help detail the transition from the region of clay minerals to the one dominated by sulfates.

-

-  Because it's winter at Curiosity's location, the skies in the new panorama are relatively dust-free, providing a clear view all the way down to Gale Crater's floor.  Curiosity has driven 16 miles so far during the mission.

-

-   Curiosity has already started up a path winding between "Rafael Navarro Mountain," recently nicknamed to honor a deceased mission scientist, and a towering butte that's taller than a four-story building. 

-

-  In the year 2021, the rover will drive past these two features into a narrow canyon before revisiting the "Greenheugh Pediment," a slope with a sandstone cap that the rover briefly summited last year.

-

-  August 18, 2021     CURIOSITY  - the rover on Mars?              3251                                                                                                                                                      

----------------------------------------------------------------------------------------

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--  email feedback, corrections, request for copies or Index of all reviews 

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Wednesday, August 18, 2021  ---------------------------






3250 - ASTEROIDS - Bennu and what killed dinosaurs?

 -  3250   -  ASTEROIDS  -  Bennu and what killed dinosaurs?  Asteroid Bennu is one of the two most hazardous known asteroids in our Solar System. The OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer) spacecraft orbited Bennu for more than two years and gathered data that has allowed scientists to better understand the asteroid’s future orbit, trajectory and Earth-impact probability.


 ------------------  3250  -   ASTEROIDS  -  Bennu and what killed dinosaurs?

-

-  In the most precise calculations of an asteroid’s trajectory ever made, researchers determined Bennu’s total impact probability through the year 2300 is about 1 in 1,750 (or 0.057%). 

-

-  The asteroid will make a close approach to Earth in 2135.    Earth’s gravity will alter the asteroid’s path, and on September 24, 2182 as the date of a potential impact, with an impact probability of 1 in 2,700 (or about 0.037%).  There is a 99.94% probability that Bennu is NOT on an impact trajectory.

-

-   Bennu was first discovered in 1999.   Since its discovery, Bennu has been extensively tracked with 580 ground-based optical astrometric observations. The asteroid made three relatively close passes of Earth in 1999, 2005, and 2011, during which the Arecibo and Goldstone radar stations collected a wealth of data about Bennu’s motion.

-

-  OSIRIS-REx discovered particles being ejected from asteroid Bennu shortly after arriving at the asteroid.   Its two-year reconnaissance and sample collection has provided crucial data about the 500-meter-wide asteroid.

-

-   Scientists expected Bennu’s surface to be smooth and sandy, but the first images from OSIRIS-REx revealed a rugged boulder-field, littered with large rocks and loose gravel. 

-

-  The asteroid was expected to be geologically quiet, but just six days after arriving in orbit, the spacecraft observed the asteroid ejecting bits of rock, due to rocks on the asteroid cracking because of the day-night heat cycle. 

-

-   Bennu even has pieces of “Vesta” on it. This spacecraft scooped up a sample of rock and dust from the asteroid’s surface in October of 2020, which it will deliver to Earth on September 24, 2023.

-

-   The researchers took into account all kinds of small influences, including the tiny gravitational pull of more than 300 other asteroids, and the drag caused by interplanetary dust. They even checked to see if OSIRIS-REx pushed the asteroid off course when the spacecraft briefly touched its rocky surface with its Touch-And-Go (TAG) sample collection maneuver. But that event had a negligible effect.

-

-  The researchers especially focused on a phenomenon called the “Yarkovsky effect“, where an object in space would, over long periods of time, be noticeably nudged in its orbit by the slight push created when it absorbs sunlight and then re-emits that energy as heat. 

-

-  Over short timeframes, this thrust is minuscule, but over long periods, the effect on the asteroid’s position builds up and can play a significant role in changing an asteroid’s path.

-

-  The Yarkovsky effect will act on all asteroids of all sizes, and while it has been measured for a small fraction of the asteroid population from afar   The effect on Bennu is equivalent to the weight of three grapes constantly acting on the asteroid, tiny, yes, but significant when determining Bennu’s future impact chances over the decades and centuries to come. 

-

-  The spacecraft is now returning home, carrying a precious sample from this fascinating ancient object that will help us better understand not only the history of the solar system but also the role of sunlight in altering Bennu’s orbit since we will measure the asteroid’s thermal properties at unprecedented scales in laboratories on Earth when it arrives.

-

-  The Earth has experienced very many asteroids in the past.  One of the most famous is the asteroid credited with the extinction of the dinosaurs 66,000,000 years ago.  This asteroid is likely to have originated from the outer half of the solar system’s main asteroid belt. 

-

-  Known as the “Chicxulub impactor“, this large asteroid has an estimated width of 6 miles and produced a crater in Mexico’s Yucatan peninsula that spans 90 miles . 

-

-  After its sudden contact with Earth, the asteroid wiped out not only the dinosaurs, but around 75 percent of the planet’s animal species. It is widely accepted that this explosive force created was responsible for the mass extinction that ended the “Mesozoic era“.

-

-  Observations of 130,000 model asteroids, along with data and behavior seen in other known impactors, found that objects are 10 times more likely to reach Earth from the outer asteroid belt than previously thought. 

-

-  Prior to crashing into Earth, the extinction-causing asteroid orbited the sun with others, in the main asteroid belt. This concentrated band lies between planets Mars and Jupiter, with its contents usually kept in place by the forces of gravity. 

-

-   Researchers discovered that “escape hatches” could be created by thermal forces, which pull more distant asteroids out of orbit and in the direction of Earth. 

-

-  The objects found in these outermost parts of the asteroid belt include many carbonaceous chondrite impactors. These are dark, porous and carbon-containing rocks which can also be found on Earth. 

-

-  Geologists discovered that the Chicxulub asteroid had a similar composition to today’s carbonaceous chondrites.  In the solar system, many objects surrounding Earth share similar composition to this impactor, however they are all much smaller, with widths around one mile.

-

-  By looking at wide timescales of the Chicxulub asteroid, the scientists could predict that a 6-mile asteroid is likely to come into contact with Earth once every 250 million years. Their model showed almost 50 percent of these significant impactors to be of the same carbonaceous chondrite composition. 

-

-  Get ready for the next one.

-

-  August 17, 2021    ASTEROIDS  -  Bennu and what killed dinosaurs?      3201                                                                                                                                                      

----------------------------------------------------------------------------------------

-----  Comments appreciated and Pass it on to whomever is interested. ---- 

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--  email feedback, corrections, request for copies or Index of all reviews 

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Wednesday, August 18, 2021  ---------------------------